Tunnelling of relativistic particles from new type black hole in new massive gravity

Gecim G., SUCU Y.

JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, cilt.2013, sa.2, 2013 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 2013 Sayı: 2
  • Basım Tarihi: 2013
  • Doi Numarası: 10.1088/1475-7516/2013/02/023
  • Dergi Adı: JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Anahtar Kelimeler: modified gravity, gravity, quantum field theory on curved space, HAWKING RADIATION, SELF-INTERACTION, DIRAC PARTICLES, TEMPERATURE, EQUATION, CREATION
  • Akdeniz Üniversitesi Adresli: Evet

Özet

In the framework of the three dimensional New Massive Gravity theory introduced by Bergshoeff, Hohm and Townsend, we analyze the behavior of relativistic spin-1/2 and spin-0 particles in the New-type Black Hole backgroud, solution of the New Massive Gravity. We solve Dirac equation for spin-1/2 and Klein-Gordon equation for spin-0. Using Hamilton-Jacobi method, we discuss tunnelling probability and Hawking temperature of the spin-1/2 and spin-0 particles for the black hole. We observe that the tunnelling probability and Hawking temperature are same for the spin-1/2 and spin-0.

In the framework of the three dimensional New Massive Gravity theory introduced by Bergshoeff, Hohm and Townsend, we analyze the behavior of relativistic spin-1/2 and spin-0 particles in the New-type Black Hole backgroud, solution of the New Massive Gravity.We solve Dirac equation for spin-1/2 and Klein-Gordon equation for spin-0. Using Hamilton-Jacobi method, we discuss tunnelling probability and Hawking temperature of the spin-1/2 and spin-0 particles for the black hole. We observe that the tunnelling probability and Hawking temperature are same for the spin-1/2 and spin-0.